Light scattering due to particulate contamination over the primary mirror of Visible Emission Line Coronagraph on board Aditya-L1 mission

2021 ◽  
Vol 60 (07) ◽  
Author(s):  
Suresh Venkata ◽  
Raghavendra Prasad Budihal
2013 ◽  
Vol 42 (2) ◽  
pp. 96-100 ◽  
Author(s):  
Jagdev Singh ◽  
Raja Bayanna ◽  
K. Sankarasubramanian

2019 ◽  
Vol 64 (7) ◽  
pp. 1455-1464
Author(s):  
Jagdev Singh ◽  
B. Raghavendra Prasad ◽  
Suresh Venkata ◽  
Amit Kumar

2018 ◽  
Vol 45 (2) ◽  
pp. 219-229 ◽  
Author(s):  
N. Raj Kumar ◽  
B. Raghavendra Prasad ◽  
Jagdev Singh ◽  
Suresh Venkata

2017 ◽  
Vol 3 (1) ◽  
pp. 014002 ◽  
Author(s):  
Suresh N. Venkata ◽  
B. Raghavendra Prasad ◽  
Raj Kumar Nalla ◽  
Jagdev Singh

1996 ◽  
Vol 39 (2) ◽  
pp. 42-48
Author(s):  
Aleck Lee ◽  
Michael Fong

This paper presents an analysis of light scattering by surface particles on the sensor window of a missile during ascent flight. The particulate contaminant distribution on the window is calculated by tallying the number of particles in a set of size ranges. The particulate contamination at the end of the mission is predicted by adding the contributions from the events of ground and flight operations. The surface particle redistribution caused by vibroacoustic-induced surface acceleration was found to contribute the most to particulate surface contamination. The analytical surface obscuration calculation with a set of particle counts was compared with the results of the image analyzer measurement. The analytical results, which were calculated with a given function of particle shape depending on size, were more conservative than the measurement. A scattering calculation using a verified BSDF model showed that the scattering was less than 0.001 at 20 deg off the direction of the incident light in the mid IR wavelength when the surfaces were at Level 300 initially.


2017 ◽  
Vol 13 (S335) ◽  
pp. 340-343 ◽  
Author(s):  
D. Banerjee ◽  
R. Patel ◽  
V. Pant ◽  

AbstractVisible Emission Line Coronagraph (VELC) on board ADITYA-L1 is an internally occulted coronagraph with mirror as its primary objective element. It has a field of view (FOV) starting from 1.05 R⊙– 3 R⊙. It will observe the corona in continuum centered at 5000 Å and will perform spectroscopic observations of inner corona in two visible (5303 Å and 7892 Å) and one infrared (10747 Å) wavelengths. VELC will be capable of observingthecorona with high spatial and temporal resolutions. We present an overview of the inner coronagraph (VELC) design and introduce the concept of an on-board automated coronal mass ejections (CMEs) detection logic proposed for this payload.


2018 ◽  
Vol 13 (S340) ◽  
pp. 171-172
Author(s):  
Ritesh Patel ◽  
K. Amareswari ◽  
Vaibhav Pant ◽  
Dipankar Banerjee ◽  
K. Sankarasubramanian

AbstractAn onboard automated coronal mass ejections (CMEs) detection algorithm has been developed for Visible Emission Line Coronagraph (VELC) onboard ADITYA-L1. The aim of this algorithm is to reduce the load on telemetry by sending the high spatial (~ 2.51 arcsec pixel−1) and temporal (1 s) resolution images of corona from 1.05 R⊙ to 3 R⊙, containing CMEs and rejecting others. It is based on intensity thresholding followed by an area thresholding in successive running difference images which are re-binned to lower resolution to improve signal to noise. Here we present the results of application of the algorithm on synthetic corona images generated for the VELC field of view (FOV).


2017 ◽  
Vol 113 (04) ◽  
pp. 613 ◽  
Author(s):  
B. Raghavendra Prasad ◽  
Dipankar Banerjee ◽  
Jagdev Singh ◽  
S. Nagabhushana ◽  
Amit Kumar ◽  
...  

Solar Physics ◽  
2018 ◽  
Vol 293 (7) ◽  
Author(s):  
Ritesh Patel ◽  
Amareswari K ◽  
Vaibhav Pant ◽  
Dipankar Banerjee ◽  
Sankarasubramanian K. ◽  
...  

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